DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 NGC 5174 202.3569 11.0203 201.73681 11.278322 196.356635 18.897363 333.76702191 71.58014685 102.4436 55219.0472685185 2010-01-23 01:08:04 55220.5835532407 2010-01-24 14:00:19 804048010 54.5151 50 54.5231 54.5151 0 54.5231 2 2 0 2 1 0 0 44.0362 44.0362 132.6979 0 PROCESSED 57550.3479050926 2016-06-11 08:20:59 55595 2011-02-03 00:00:00 55229.1361226852 2010-02-02 03:16:01 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041504 Galaxies are missing most of their baryons when compared to the cosmological baryon to dark matter ratio: the Milky Way retained only 30% of its baryons while lower mass galaxies retain less than 10%. Probably, these baryons were expelled by intense galactic winds during the early star formation period at z = 1-3. These galactic winds can carry gas far beyond the virial radius of small and modest galaxies, but the most massive galaxies should retain much of this gas. We propose to test this picture by searching for the missing baryons surrounding two extremely massive spiral galaxies, with 6-8 times the stellar content of M31 and with v_rot = 370, 420 km/s. If successful, we will detect a significant fraction of the 3-4E11 Msun of the missing baryons as hot gas. EXTRAGALACTIC DIFFUSE SOURCES 8 C JOEL BREGMAN USA 4 AO4 THE BARYON CONTENT OF MASSIVE SPIRAL GALAXIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804048010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804048010'

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